Yeah I already understood that part, but it's still funny when it happens and it's always stuns me a bit :D

I wouldn't go that far in a universe where "history of the entire world, i guess" exists. But thanks, I'm blushed

@@KofteistKofteEN The very early universe The first picosecond (10−12) of cosmic time includes the Planck epoch, during which currently established laws of physics may not have applied; the emergence in stages of the four known fundamental interactions or forces-first gravitation, and later the electromagnetic, weak and strong interactions; and the accelerated expansion of the universe due to cosmic inflation. Tiny ripples in the universe at this stage are believed to be the basis of large-scale structures that formed much later. Different stages of the very early universe are understood to different extents. The earlier parts are beyond the grasp of practical experiments in particle physics but can be explored through the extrapolation of known physical laws to extreme high temperatures. The early universe This period lasted around 370,000 years. Initially, various kinds of subatomic particles are formed in stages. These particles include almost equal amounts of matter and antimatter, so most of it quickly annihilates, leaving a small excess of matter in the universe. At about one second, neutrinos decouple; these neutrinos form the cosmic neutrino background (CνB). If primordial black holes exist, they are also formed at about one second of cosmic time. Composite subatomic particles emerge-including protons and neutrons-and from about 2 minutes, conditions are suitable for nucleosynthesis: around 25% of the protons and all the neutrons fuse into heavier elements, initially deuterium which itself quickly fuses into mainly helium-4. By 20 minutes, the universe is no longer hot enough for nuclear fusion, but far too hot for neutral atoms to exist or photons to travel far. It is therefore an opaque plasma. The recombination epoch begins at around 18,000 years, as electrons are combining with helium nuclei to form He+ . At around 47,000 years,[2] as the universe cools, its behavior begins to be dominated by matter rather than radiation. At around 100,000 years, after the neutral helium atoms form, helium hydride is the first molecule. Much later, hydrogen and helium hydride react to form molecular hydrogen (H2) the fuel needed for the first stars. At about 370,000 years,[3][4][5][6] neutral hydrogen atoms finish forming ("recombination"), and as a result the universe also became transparent for the first time. The newly formed atoms-mainly hydrogen and helium with traces of lithium-quickly reach their lowest energy state (ground state) by releasing photons ("photon decoupling"), and these photons can still be detected today as the cosmic microwave background (CMB). This is the oldest direct observation we currently have of the universe.

Yeah, after some technical projects, I'm planing to do a much more deeper dive on magic and especially Botania (for that sweet sweet armor and trinkets... But before that, we have some interesting projects and everything becomes much more interesting after 19th episode on the technical side :)

+ scan every single crafting material cuz aspects!

It is a given that you should scan every single new thing you made in this pack, if you want to dive deep into the thaumcraft.

This video is still 2.5.1. I'll switch to 2.6.0 on 23th episode if I remember correctly.

@@KofteistKofteEN why specially 23th ? we are in 14

Because of the backlog...

@@KofteistKofteEN hmm okey, Kofte,i have a problem,are there any platform to explain face to face with you? it is about your dc channel.

you can dm me on discord